Intermittent heating in the solar corona employing a 3D MHD model

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Bingert, S ^a,b   Peter, H ^a,b  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

Author keywords

magnetohydrodynamics (MHD); methods: numerical; stars: coronae; Sun: corona

Indexed keywords

COOL STARS; CURRENT SHEETS; HEATING MECHANISMS; INTERMITTENT HEATING; MAGNETIC FIELD LINE; MAGNETIC STRESS; METHODS: NUMERICAL; MHD MODELS; NANOFLARES; OHMIC DISSIPATION; PHOTOSPHERIC MOTIONS; RADIATIVE LOSS; SOLAR CORONA; SPITZER; STARS: CORONAE; SUN: CORONA; TEMPORAL EVOLUTION; TIME AND SPACE; TRANSITION REGIONS;

HEATING; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; POWER QUALITY; STARS;

THREE DIMENSIONAL;

EID: 79956364104     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016019     Document Type: Article

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